Astrophysics

    

A Thermodynamic Degree of Freedom Solution to the Galaxy Cluster Problem of Mond

Authors: E.P.J. de Haas

In this paper I discus the degree of freedom parameter of the emergent Dark Matter force. I show how this degree of freedom parameter N results in a possible difference between observed mass and apparent mass, in cases where N is larger than one. This might solve the galaxy cluster mass discrepancy of MOND. In my model the degrees of freedom of galaxies in clusters influences their number of microstates inside the cluster and thus their entropy. And then it also influences the apparent baryonic mass in the emergent Dark Matter force, a mass that will appear a factor in between two or three bigger than can be directly observed.

Comments: 5 Pages.

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Submission history

[v1] 2015-10-22 18:07:49

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